411 REFERENCE · Wikipedia
19521 Chaos
Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.
Classical Kuiper belt object
October 2019
yes #C2E0FF 19521 Chaos 24px (astrological) Deep Ecliptic Survey 19 November 1998 17 October 1991 19521-chaos hst.jpg 19521 Chaos as imaged by the Hubble Space Telescope in September 2001 (19521) Chaos ˈ k eɪ . ɒ s 1998 WH 24 Chaotian k eɪ ˈ oʊ ʃ ən Chaos TNO (cubewano) 13 January 2016 (JD 2457400.5) 5902 days (16.16 yr) 2 12.5 AU Tm on 35.8 AU Tm on 5.884 45.796 AU Tm on 40.957 AU Tm on ≈ 23 December 2033JPL Horizons Observer Location: @sun (Perihelion occurs when deldot changes from negative to positive. Uncertainty in time of perihelion is 3-sigma.)±10 days 50.636 AU Tm on on 0.10567 309.92 yr (113199 d) 12.0502° 50.0239° 58.4097° 337.2998° 4.3931 km/s 1? (compact or contact binary) 415 83 30 km equivalentJosé María Gómez-Limón Gallardo et al. (2024) New evidence that (19521) Chaos might be a large compact binary600 140 130 km665 ~ B–V=0.95 0.03V–R=0.63 0.03V–I=1.25 0.04 4.64<ref
name=jpldata/>5.0 0.1 (calculated) 0.00318023 ms / day
19521 Chaos (provisional designation 1998 WH 24) is a cubewano, a Kuiper belt object not in resonance with any planet. Chaos was discovered in 1998 by the Deep Ecliptic Survey with Kitt Peak's 4 m telescope.
Occultations suggest it is a compact or contact binary equivalent to a sphere 400 to 500 km in diameter. On 20 November 2020, Chaos occulted a magnitude 16.8 star. Three observers detected the occultation, finding that the object is likely smaller than 600 km in diameter. Another occultation was recorded on 14 January 2022; full results on size, shape, geometric albedo, and the spin-axis orientation have not been released.February 2023 A further occultation occurred on 28 September 2023, with a shadow crossing most of North America. This occultation was observed by over 30 observers;Gault Dave OccultWatcher Cloud https://cloud.occultwatcher.net/event/1000-19521-87528-649970-U028826/1103807 OccultWatcher 29 September 2023
preliminary analysis suggests that Chaos is a binary (possibly a contact binary).https://ui.adsabs.harvard.edu/abs/2023pses.conf80462G/abstract 2023pses.conf80462G Chaos: Stellar Occultations Reveal a Binary Tno? Gómez-Limón Gallardo José María Leiva R. Ortiz J. L. Desmars J. Kilic Y. Vara-Lubiano M. Santos-Sanz P. Kretlow M. Rommel F. L. Morales N. Fernandez-Valenzuela E. Souami D. Lucky Star Team Observers of Nov. 2020, Jan 2022, Dec 2022 Mar 2023 Occultations Seventh Edition of the Spanish Meeting of Planetary Sciences and Exploration of the Solar System (7Th Cpess 2023
Name
On 28 March 2002, it was named after the primeval state of existence in Greek mythology, from which the first gods appeared.
Planetary symbols are no longer much used in astronomy, so Chaos never received a symbol in the astronomical literature. There is no standard symbol for Chaos used by astrologers either. Michael Moorcock's Symbol of Chaos (16px) has occasionally been used.https://www.unicode.org/L2/L2021/21224-dwarf-planet-syms.pdf Unicode request for dwarf-planet symbols Miller Kirk 26 October 2021 unicode.org
Orbit
thumb|A recreation of the 2023 occultation
Chaos has an orbital period of approximately 309 years. Its orbit is longer, but less eccentric than the orbit of Pluto. Chaos's orbit is inclined approximately 12° to the ecliptic. Its orbit never crosses the orbit of Neptune. Currently, the closest approach possible to Neptune (MOID) is 12.5 AU e9km e9mi 3 unit on.
Chaos will come to perihelion at around December 2033, coming as close as 40 AU e9km e9mi 3 unit from Earth. Its brightest magnitude will be 20.8.
References
25em 2007-12-14 last obs
19521 Chaos (1998 WH24)
JPL Small-Body Database Browser
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=Chaos
11 April 2016
Thayer
1994
Gray World, Green Heart Wiley
9780471572732
https://archive.org/details/grayworldgreenhe00thay_0
registration
April 2020
Buie, Marc W.
Marc W. Buie
Orbit Fit and Astrometric record for 19521
2004-11-09
SwRI
Space Science Department
http://www.boulder.swri.edu/~buie/kbo/astrom/19521.html
2008-09-28 dmy-all
(19521) Chaos = 1998 WH24
IAU Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=Chaos
2018-02-10 dmy-all
"TNOs are cool": A survey of the trans-Neptunian region VI. Herschel / PACS observations and thermal modeling of 19 classical Kuiper belt objects
https://archive.org/details/arxiv-1202.3657
Vilenius, E. Kiss, C. Mommert, M.
Müller, T. Santos-Sanz, P. Pal, A.
Stansberry, J. Mueller, M. Peixinho, N.
Fornasier, S. Lellouch, E. Delsanti, A.
Thirouin, A. Ortiz, J.L. Duffard, R.
Perna, D. Szalai, N. Protopapa, S.
Henry, F. Hestroffer, D. Rengel, M.
Dotto, E. Hartogh, P. Astronomy and Astrophysics
2012
541
A94
10.1051/0004-6361/201118743
free 1204.0697v1
2012A&A...541A..94V
54222700
6
MPEC 2008-O05 : Distant Minor Planets (2008 AUG. 2.0 TT)
17 July 2008
Minor Planet Center
https://www.minorplanetcenter.net/mpec/K08/K08O05.html
2011-01-08 dmy-all
The color distribution in the Edgeworth-Kuiper Belt
A. Doressoundiram
N. Peixinho
C. de Bergh
S. Fornasier
Ph. Thébault
M.A. Barucci
C. Veillet
October 2002
The Astronomical Journal
124
4
2279–2296
10.1086/342447
astro-ph/0206468
2002AJ....124.2279D 30565926
etal
Mónica Vara-Lubiano
Nicolás Morales
Flavia Rommel
José Luis Ortiz
Bruno Sicardy
Pablo Santos-Sanz
The multi-chord stellar occultation by (19521) Chaos on 2020 November 20
https://meetingorganizer.copernicus.org/EPSC2021/EPSC2021-626.html
September 2021
15th Europlanet Science Congress 2021
Europlanet Society
EPSC2021-626
10.5194/epsc2021-626
2021EPSC...15..626V
26 June 2022 free
etal
José Luis Ortiz
Nicolás Morales
Mónica Vara-Lubiano
Mike Kretlow
Bruno Sicardy
Pablo Santos-Sanz
The Trans-Neptunian Object (19521) Chaos as seen from stellar occultations and photometry observations
https://meetingorganizer.copernicus.org/EPSC2022/EPSC2022-520.html
September 2022
16th Europlanet Science Congress 2022
Europlanet Society
EPSC2022-520
10.5194/epsc2022-520
2 January 2023 free subscription
External links
http://cfa-www.harvard.edu/mpec/J98/J98X08.html Original Minor Planet Electronic Circular (1998-X08) for 19521 Chaos
http://cfa-www.harvard.edu/mpec/J99/J99V03.html Revised Minor Planet Electronic Circular (1999-V03) 19521 Chaos
19521
19521
Category:Classical Kuiper belt objects
Category:Discoveries by the Deep Ecliptic Survey
Chaos
19981119
Chaos
Category:Long stubs with short prose